COSMOS, VOL. II - World eBook Library

COSMOS, VOL. II - World eBook Library COSMOS, VOL. II - World eBook Library

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I)] DISCOVERIES IN THE CELESTIAL SPACES. G97 being of opinion that some were higher and others lower than the rest. The idea formed of the heaven of the fixed stars was extended to the planets and thus arose the ; theory of the eccentric intercalated spheres of Eudoxus and Menoechmus, and of Aristotle, who was the inventor of retrograde spheres. The theory of epicycles, a construction which adapted itself most readily to the representation and calculation of the planetary movements, was, a century afterwards, made by the acute mind of Apollonius to supersede solid spheres. However much I may incline to mere ideal abstraction, I here refrain from attempting to decide historically whether, as Ideler believes, it was not until after the establishment of the Alexandrian Museum that " a free movement of the planets in space was regarded as possible," or whether before that period the intercalated transparent spheres t(of which there were twentyseven according to Eudoxus, and fifty-five according to Aris- totle), as well as the epicycles which passed from Hipparchus and Ptolemy to the middle ages, were regarded generally not as solid bodies of material thickness, but merely as ideal abstractions. It is more certain that in the middle of the sixteenth century, when the theory of the seventy-seven hoinocentric spheres of the learned writer, Girolamo Fracas- toro, found general approval ; and when, at a later period, the opponents of Copernicus sought all means of upholding the Ptolemaic system, the idea of the existence of solid spheres, circles, and epicycles, which was especially favoured by the Fathers of the Church, was still very widely diffused. Tycho Brahe expressly boasts that his considerations on the orbits of comets first proved the impossibility of solid spheres, and thus destroyed the artificial fabrics. He filled the free space of heaven with air, and even believed that the resisting medium when disturbed by the revolving heavenly bodies, might generate tones. The un-imaginative Rothmann believed it necessary to refute this renewed Pythagorean myth of celestial harmony. Kepler's great discovery that all the planets move round the sun in ellipses, and that the sun lies in one of the foci of these ellipses, at length freed the original Copernican system from eccentric circles and all epicycles.* The planetary structure * A better insight into the free movement of bodies, and into the independence of the direction once giveu to the earth's axis, and into the

698 COSMOS. of the world now appeared objectively, and as it were archi- tecturally, in its simple grandeur ; but it remained for Isaac Newton to disclose the play and connection of the internal forces which animate and preserve the system of the universe. We have already often remarked in the history of the gradual development of human knowledge, that important but apparently accidental discoveries, and the simultaneous appearance of many great minds, are crowded together in a short period of time ; and we find this phenomenon most of the seventeenth strikingly manifested in the first ten years century ; for Tycho Brahe (the founder of modern astronomic^ calculations), Kepler, Galileo, and Lord Bacon, were cotemporaries. All these, with the exception of Tycho Brahe, were enabled, in the prime of life, to benefit by the labours of Descartes and Fermat. The elements of Bacon's Instauratio Magna appeared in the English language in 1605, fifteen years before the Novum Organon. The invention of the telescope, and the greatest discoveries in physical astronomy (viz., Jupiter's satellites, the sun's spots, the phases of Venus, and the remarkable form of Saturn), fall between the years 1609 and 1612. Kepler's speculations on the elliptic orbit of Mars,* were began in 1601, and gave occasion, eight years after, to the completion of the work entitled Astronomia nova sett Physica celestis. " By the study of the orbit of Mars," writes " Kepler, we must either arrive at a knowledge of the secrets of astronomy, or for ever remain ignorant of them. I have succeeded, by untiring and continued labour, in subjecting the inequalities of the movement of Mars to a natural law." The generalization of the same idea led the highly- gifted mind of Kepler to the great cosmical truths and presentiments which, ten years later, he published in his work entitled Harmonices Mundi " libri quinque. I believe," he well observes in a letter to the Danish astronomer Longo- rotatory and progressive movement of the terrestrial planet in its orbit, has freed the original system of Copernicus from the assumption of a declination-movement, or a so-called third movement of the earth (De Revolut. orb. cod., lib. i. cap. 11, triplex motus telluris.) The parallelism, of the earth's axis is maintained in the annual revolution round the sun, in conformity with the law of inertia, without the application correcting epicycle. * Delambre, Hist, del'Astronomic ancienne, t. ii. p. 381. of a

I)] DISCOVERIES IN THE CELESTIAL SPACES. G97<br />

being of opinion that some were higher<br />

and others lower than<br />

the rest. The idea formed of the heaven of the fixed stars<br />

was extended to the planets and thus arose the ;<br />

theory of the<br />

eccentric intercalated spheres of Eudoxus and Menoechmus, and<br />

of Aristotle, who was the inventor of retrograde spheres. The<br />

theory of epicycles,<br />

a construction which adapted itself most<br />

readily to the representation and calculation of the planetary<br />

movements, was, a century afterwards, made by the acute<br />

mind of Apollonius to supersede solid spheres. However much<br />

I may incline to mere ideal abstraction, I here refrain from<br />

attempting to decide historically whether, as Ideler believes,<br />

it was not until after the establishment of the Alexandrian<br />

Museum that " a free movement of the planets in space was<br />

regarded as possible," or whether before that period the<br />

intercalated transparent spheres t(of which there were twentyseven<br />

according to Eudoxus, and fifty-five according to Aris-<br />

totle), as well as the epicycles which passed from Hipparchus<br />

and Ptolemy to the middle ages, were regarded generally not<br />

as solid bodies of material thickness, but merely as ideal<br />

abstractions. It is more certain that in the middle of the<br />

sixteenth century, when the theory of the seventy-seven hoinocentric<br />

spheres of the learned writer, Girolamo Fracas-<br />

toro, found general approval ; and when, at a later period,<br />

the opponents of Copernicus sought all means of upholding<br />

the Ptolemaic system, the idea of the existence of solid<br />

spheres, circles, and epicycles, which was especially favoured<br />

by the Fathers of the Church, was still very widely diffused.<br />

Tycho Brahe expressly<br />

boasts that his considerations on<br />

the orbits of comets first proved the impossibility of solid<br />

spheres, and thus destroyed the artificial fabrics. He filled<br />

the free space of heaven with air, and even believed that<br />

the resisting medium when disturbed by the revolving<br />

heavenly bodies, might generate tones. The un-imaginative<br />

Rothmann believed it necessary to refute this renewed<br />

Pythagorean myth of celestial harmony.<br />

Kepler's great discovery that all the planets move round the<br />

sun in<br />

ellipses, and that the sun lies in one of the foci of these<br />

ellipses, at length freed the original Copernican system from<br />

eccentric circles and all epicycles.* The planetary structure<br />

* A better insight into the free movement of bodies, and into the independence<br />

of the direction once giveu to the earth's axis, and into the

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